A program to calculate coronal emission line strengths
- 1 May 1977
- journal article
- Published by Elsevier in Computer Physics Communications
- Vol. 13 (1) , 25-38
- https://doi.org/10.1016/0010-4655(77)90024-8
Abstract
No abstract availableKeywords
This publication has 4 references indexed in Scilit:
- Plasma diagnostic techniques in the ultraviolet - The C III density-sensitive lines in the sunThe Astrophysical Journal, 1976
- A general program to calculate atomic continuum processes using the R-matrix methodComputer Physics Communications, 1974
- Oscillator strengths of transitions in the beryllium sequenceJournal of Physics B: Atomic and Molecular Physics, 1974
- The Ionization Equilibrium of Elements Between Carbon and NickelMonthly Notices of the Royal Astronomical Society, 1969